Inference is crucial in modern astronomical research, where hidden astrophysical features and patterns are often estimated from indirect and noisy measurements. Inferring the posterior of hidden features, conditioned on the observed measurements, is essential for understanding the uncertainty of results and downstream scientific interpretations. Traditional approaches for posterior estimation include sampling-based methods and variational inference. However, sampling-based methods are typically slow for high-dimensional inverse problems, while variational inference often lacks estimation accuracy. In this paper, we propose alpha-DPI, a deep learning framework that first learns an approximate posterior using alpha-divergence variational inference paired with a generative neural network, and then produces more accurate posterior samples through importance re-weighting of the network samples. It inherits strengths from both sampling and variational inference methods: it is fast, accurate, and scalable to high-dimensional problems. We apply our approach to two high-impact astronomical inference problems using real data: exoplanet astrometry and black hole feature extraction.
翻译:在现代天文研究中,隐蔽的天体物理特征和模式往往是从间接和吵闹的测量中估计出来的,推断以观测到的测量结果为条件的隐蔽特征的后部,对于了解结果的不确定性和下游科学解释至关重要。传统的后部估计方法包括基于取样的方法和变异推论。但是,对于高维反向问题,基于取样的方法通常比较缓慢,而差异推论往往缺乏估计准确性。在本文中,我们提出了一个深层次学习框架,首先用基因神经网络对准一个近似后部,然后通过网络样品的重要重新加权产生更准确的远部样本。它从取样和变异推论方法中继承了优势:它快速、准确和可伸缩到高度问题。我们用真实数据将我们的方法应用于两个高影响天文推论问题:外观测量和黑洞地特征提取。